Fig. 13

Convergence of secular angles Ω and ϖ of Datura members to the largest fragment (1270) Datura. The histograms show number of converging trials in the past regrouped into 10 kyr bins: (i) light gray for a cut-off limit δV< 5 m s-1; (ii) the dark gray for a cut-off limit δV< 2 m s-1. Each time the histograms were normalized to unity for the first case. Left and middle columns for asteroids on stable orbits away from the M9/16 mean motion resonance. The right column for objects that either currently reside in this resonance (89309, 433382 and 2009 VS116), or the extreme member that jumped over this resonance (452713).
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